Nuclear equation of state from observations of short gamma-ray burst remnants

P.D. Lasky, B. Haskell, V. Ravi, Eric Howell, David Coward

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    101 Citations (Scopus)


    The favored progenitor model for short γ-ray bursts (SGRBs) is the merger of two neutron stars that triggers an explosion with a burst of collimated γ-rays. Following the initial prompt emission, some SGRBs exhibit a plateau phase in their X-ray light curves that indicates additional energy injection from a central engine, believed to be a rapidly rotating, highly magnetized neutron star. The collapse of this "protomagnetar" to a black hole is likely to be responsible for a steep decay in X-ray flux observed at the end of the plateau. In this paper, we show that these observations can be used to effectively constrain the equation of state of dense matter. In particular, we show that the known distribution of masses in binary neutron star systems, together with fits to the X-ray light curves, provides constraints that exclude the softest and stiffest plausible equations of state. We further illustrate how a future gravitational wave observation with Advanced LIGO/Virgo can place tight constraints on the equation of state, by adding into the picture a measurement of the chirp mass of the SGRB progenitor. © 2014 American Physical Society.
    Original languageEnglish
    Article number047302
    Pages (from-to)047302-1 - 047302-5
    Number of pages5
    JournalPhysical Review D - Particles, Fields, Gravitation and Cosmology
    Issue number4
    Publication statusPublished - 26 Feb 2014


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